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The Problem of Critical Inclination Combined with a Resonance in Mean Motion in Artificial Satellite Theory

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Qualitative and Quantitative Behaviour of Planetary Systems

Abstract

In this paper, the problem of a geosynchronous artificial satellite orbiting near the critical inclination is investigated. At the critical inclination the secular J 2 effect in the argument of perigee is zero. This allows the apogee to be stabilized above the desired (e.g. northern European) coverage area by adjusting other orbital elements, thus providing a greatly enhanced coverage of the target regions. Apart from the improved visibility from high-latitude-regions, highly inclined orbits are becoming attractive due to the increasing collision hazard of geostationary satellites with debris and de-activated spacecrafts which “pollute” the relatively confined geostationary ring.

Reaearch Assisitant for the Belgian National Fund for Scientific Reaearch

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© 1993 Springer Science+Business Media Dordrecht

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Delhaise, F., Henrard, J. (1993). The Problem of Critical Inclination Combined with a Resonance in Mean Motion in Artificial Satellite Theory. In: Dvorak, R., Henrard, J. (eds) Qualitative and Quantitative Behaviour of Planetary Systems. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-2030-2_25

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  • DOI: https://doi.org/10.1007/978-94-011-2030-2_25

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-4898-9

  • Online ISBN: 978-94-011-2030-2

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